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FOR IMMEDIATE RELEASE
August 24, 2004

Network of Small Telescopes Discovers Distant Planet

Flagstaff, AZ—Fifteen years ago, the largest telescopes in the world had yet to locate a planet orbiting another star. Today telescopes no larger than those available in department stores are proving capable of spotting previously unknown worlds. A newfound planet detected by a small, 4-inch-diameter telescope demonstrates that we are at the cusp of a new age of planet discovery. Soon, new worlds may be located at an accelerating pace, bringing the detection of the first Earth-sized world one step closer.

"This discovery demonstrates that even humble telescopes can make huge contributions to planet searches," says Guillermo Torres of the Harvard-Smithsonian Center for Astrophysics (CfA), a co-author on the study.

This is the first extrasolar planet discovery made by a dedicated survey of many thousands of relatively bright stars in large regions of the sky. It was made using the Trans-Atlantic Exoplanet Survey (TrES), a network of small, relatively inexpensive telescopes designed to look specifically for planets orbiting bright stars. A team of scientists co-led by Edward Dunham of Lowell Observatory, Timothy Brown of NCAR, and David Charbonneau (CfA), developed the TrES network. The network's telescopes are located in Palomar Observatory (California, USA), Lowell Observatory (Arizona, USA), and the Canary Islands (Spain).

"The advantage of working as a network is that we can 'stretch the night' and monitor our fields for a longer time, increasing our chance of discovering a planet," says Georgi Mandushev (Lowell Observatory), a co-author of the paper.

This research study will be posted online at http://arxiv.org/abs/astro-ph/0408421 and will appear in an upcoming issue of The Astrophysical Journal Letters.

"It took several Ph.D. scientists working full-time to develop the data analysis methods for this search program, but the equipment itself uses simple, off-the-shelf components," says co-author David Charbonneau (CfA/Caltech).

Although the small telescopes of the TrES network made the initial discovery, follow-up observations at other facilities were required. Observations at the W. M. Keck Observatory which operates the world’s two largest telescopes in Hawaii for the University of California, Caltech, and NASA, were particularly crucial in confirming the planet’s existence.

Planet Shadows

The newfound planet is a Jupiter-sized gas giant orbiting a star located about 500 light years from the Earth in the constellation Lyra. This world circles its star every 3.03 days at a distance of only 4 million miles (6 million kilometers), much closer and faster than the planet Mercury in our solar system.

Although such planets are relatively common, astronomers used an uncommon technique to discover it. This world was found by the "transit method," which looks for a dip in a star’s brightness when a planet crosses directly in front of the star and casts a shadow. A Jupiter-sized planet blocks only about 1/100th of the light from a Sun-like star, but that is enough to make it detectable.

"This Jupiter-sized planet was observed doing the same thing that happened in June when Venus moved across (or transited) the face of our Sun," says Mandushev. "The difference is that this planet is outside our solar system, roughly 500 light years away."

To be successful, transit searches must examine many stars because we only see a transit if a planetary system is located nearly edge-on to our line of sight. A number of different transit searches currently are underway. Most examine limited areas of the sky and focus on fainter stars because they are more common, thereby increasing the chances of finding a transiting system. However the TrES network concentrates on searching brighter stars in larger swaths of the sky because planets orbiting bright stars are easier to study directly.

"All that we have to work with is the light that comes from the star," says Tim Brown (NCAR), a study co-author. "It’s much harder to learn anything when the stars are faint."

Most known extrasolar planets were found using the "Doppler method," which detects a planet’s gravitational effect on its star by looking for shifts in the star's spectrum, or rainbow of colors. However, the information that can be gleaned about a planet using the Doppler method is limited. For example, only a lower limit to the mass can be determined because the angle at which we view the system is unknown. A high-mass brown dwarf whose orbit is highly inclined to our line of sight produces the same signal as a low-mass planet that is nearly edge-on.

"When astronomers find a transiting planet, we know that its orbit is essentially edge-on, so we can calculate its exact mass. From the amount of light it blocks, we learn its physical size. In one instance, we’ve even been able to detect and study a giant planet’s atmosphere," says Charbonneau.

Sorting Suspects

The TrES survey examined approximately 12,000 stars in 36 square degrees of the sky (about half of the size of the bowl of the Big Dipper) in the constellation of Lyra. Roi Alonso (IAC), a graduate student of Brown’s, identified 16 possible candidates for planet transits. "The TrES survey gave us our initial line-up of suspects. Then, we had to make a lot of follow-up observations to eliminate the imposters," says co-author Alessandro Sozzetti (University of Pittsburgh/CfA).

After compiling the list of candidates in late April, the researchers used telescopes at CfA’s Whipple Observatory in Arizona, Oak Ridge Observatory in Massachusetts, and Lowell Observatory in Arizona to obtain additional photometric (brightness) observations, as well as spectroscopic observations that eliminated eclipsing binary stars.

In a matter of two month’s time, the team had zeroed in on the most promising candidate. High-resolution spectroscopic observations by Torres and Sozzetti using time provided by NASA on the 10-meter-diameter Keck I telescope in Hawaii clinched the case.

"Without this follow-up work the photometric surveys can’t tell which of their candidates are actually planets. The proof of the pudding is a spectroscopic orbit for the parent star. That’s why the Keck observations of this star were so important in proving that we had found a true planetary system," says co-author David Latham (CfA).

Remarkably Normal

The planet, called TrES-1, is much like Jupiter in mass and size. It is likely to be a gas giant composed primarily of hydrogen and helium, the most common elements in the Universe. But unlike Jupiter, it orbits very close to its star, giving it a temperature of around 1500 degrees F.

Astronomers are particularly interested in TrES-1 because its structure agrees so well with theory, in contrast to the first discovered transiting planet, HD 209458b. The latter world contains about the same mass as TrES-1, yet is around 30% larger in size. Even its proximity to its star and the accompanying heat don’t explain such a large size.

"Finding TrES-1 and seeing how normal it is makes us suspect that HD 209458b is an ‘oddball’ planet," says Charbonneau.

TrES-1 orbits its star every 72 hours, placing it among a group of similar planets known as "hot Jupiters." Such worlds likely formed much further away from their stars and then migrated inward, sweeping away any other planets in the process. The many planetary systems found to contain hot Jupiters indicate that our solar system may be unusual for its relatively quiet history.

Both the close orbit of TrES-1 and its migration history make it unlikely to possess any moons or rings. Nevertheless, astronomers will continue to examine this system closely because precise photometric observations may detect moons or rings if they exist. In addition, detailed spectroscopic observations may give clues to the presence and composition of the planet’s atmosphere.

The paper, "TrES-1: The Transiting Planet of a Bright K0V Star," descibing these results is authored by: Roi Alonso (IAC); Timothy M. Brown (NCAR); Guillermo Torres and David W. Latham (CfA); Alessandro Sozzetti (University of Pittsburgh/CfA); Georgi Mandushev (Lowell Observatory), Juan A. Belmonte (IAC); David Charbonneau (CfA/Caltech); Hans J. Deeg (IAC); Edward W. Dunham (Lowell Observatory); Francis T. O’Donovan (Caltech); and Robert Stefanik (CfA).

The W.M. Keck Observatory is operated by the California Association for Research in Astronomy, a scientific partnership of the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration (NASA).

Funding for the research that led to this planet's discovery was provided by NASA's Origins of Solar Systems Program.


content/release_supplements/tres1_final.jpg

New planet TrES-1 in a computer-illustrated simulation with its parent star. The K-type star is active, slightly cooler and smaller than the Sun, and likely has numerous spots and atmospheric phenomena such as flares and prominences. The planet is about 10 times closer to its star than Mercury is to the Sun. The star's radiation at this distance is intense enough so that light gases such as hydrogen may be blown away from the planet. The planet itself is a Jupiter-like giant gas planet. Credit:Jeffrey Hall, Lowell Observatory
Download a print-quality JPEG of the above image [813 KB].


content/release_supplements/tres1-2_final.jpg

Planet TrES-1 is seen here from its night side, with its parent star in the distance. In this computer-illustrated simulation, the planet looks larger than the star because we are very close to it. In reality, the star is some eight times larger than the planet. A hypothetical faint stream of hot gas is seen again in the planet's dark bulk; the star's radiation strikes the planet with roughly 100 times the intensity of the Sun's radiation at Earth, and may cause light gases to stream out behind the planet. Credit: Jeffrey Hall, Lowell Observatory.
Download a print-quality JPEG of the above image [679 KB].


content/release_supplements/tres1_transit_still.jpg

In this 20-second computer-rendered animation, planet TrES-1 is seen transiting the surface of its parent star. The planet is visible at the start of the animation near lower left, as a thin crescent. As it transits, it appears as a dark circle eclipsing part of the star's disk. The corresponding drop in brightness as the transit occurs was noted and measured by the TrES researchers, who used the parameters of the transit to determine the planet's characteristics. In real life the transit lasts slightly less than three hours. Credit: Jeffrey Hall, Lowell Observatory.
Download the AVI [82 KB].

About Lowell Observatory

Lowell Observatory is a private, non-profit research institution founded in 1894 by Percival Lowell. The Observatory has been the site of many important findings including the discovery of the large recessional velocities (redshift) of galaxies by Vesto Slipher in 1912-1914 (a result that led ultimately to the realization the universe is expanding), and the discovery of Pluto by Clyde Tombaugh in 1930. Today, Lowell's 19 astronomers use ground-based telescopes around the world, telescopes in space, and NASA planetary spacecraft to conduct research in diverse areas of astronomy and planetary science. The Observatory welcomes about 80,000 visitors each year to its Mars Hill campus in Flagstaff, Arizona for a variety of tours, telescope viewing, and special programs. Lowell Observatory currently has four research telescopes at its Anderson Mesa dark sky site east of Flagstaff, and is building a 4-meter class research telescope, the Discovery Channel Telescope.

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